scholarly journals Evidence from K2 for Rapid Rotation in the Descendant of an Intermediate-mass Star

2017 ◽  
Vol 841 (1) ◽  
pp. L2 ◽  
Author(s):  
J. J. Hermes ◽  
Steven D. Kawaler ◽  
A. D. Romero ◽  
S. O. Kepler ◽  
P.-E. Tremblay ◽  
...  
Keyword(s):  
Mass Star ◽  
Intermediate Mass ◽  
Rapid Rotation ◽  
Intermediate Mass Star

scholarly journals AN EXTENSIVE, SENSITIVE SEARCH FOR SiO MASERS IN HIGH- AND INTERMEDIATE-MASS STAR-FORMING REGIONS

2009 ◽  
Vol 691 (1) ◽  
pp. 332-341 ◽  
Author(s):  
Luis A. Zapata ◽  
Karl Menten ◽  
Mark Reid ◽  
Henrik Beuther
Keyword(s):  
Mass Star ◽  
Intermediate Mass ◽  
Star Forming ◽  
Star Forming Regions ◽  
Intermediate Mass Star

scholarly journals Low and intermediate mass star yields

2006 ◽  
Vol 450 (2) ◽  
pp. 509-521 ◽  
Author(s):  
M. Gavilán ◽  
M. Mollá ◽  
J. F. Buell
Keyword(s):  
Mass Star ◽  
Intermediate Mass ◽  
Intermediate Mass Star

scholarly journals THE INTERMEDIATE-MASS STAR-FORMING REGION LYNDS 1340. AN OPTICAL VIEW

2016 ◽  
Vol 822 (2) ◽  
pp. 79 ◽  
Author(s):  
Mária Kun ◽  
Attila Moór ◽  
Elza Szegedi-Elek ◽  
Bo Reipurth
Keyword(s):  
Mass Star ◽  
Intermediate Mass ◽  
Star Forming ◽  
Intermediate Mass Star

scholarly journals Through the AGB towards a Planetary: A hydrodynamical simulation

1997 ◽  
Vol 180 ◽  
pp. 368-368 ◽  
Author(s):  
M. Steffen ◽  
D. Schönberner ◽  
K. Kifonidis ◽  
J. Stahlberg
Keyword(s):  
Dynamical Evolution ◽  
Spherical Shape ◽  
Radiation Hydrodynamics ◽  
Mass Star ◽  
Intermediate Mass ◽  
Hydrodynamical Simulation ◽  
Two Component ◽  
Self Consistent ◽  
Intermediate Mass Star ◽  
Single Size

Based on the mass-loss description developed by Blöcker (1995, A&A, 297, 727), we present first exploratory computations of the dynamical evolution of a dusty stellar wind envelope around an intermediate mass star during the last 300 000 years on the AGB and its transformation into a planetary nebula during the following 5 000 years of post-AGB evolution. To model the dynamics of the cool dusty envelope, we used a two-component (gas/dust) 1D radiation hydrodynamics code which computes the radiation pressure on dust grains and the structure of the envelope in a self-consistent way, including the variable frictional coupling between dust and gas. The grains are either carbon or oxygen based and of single size and spherical shape.

scholarly journals A SAMPLE OF INTERMEDIATE-MASS STAR-FORMING REGIONS: MAKING STARS AT MASS COLUMN DENSITIES <1 g cm–2

2010 ◽  
Vol 140 (2) ◽  
pp. 462-479 ◽  
Author(s):  
K. Arvidsson ◽  
C. R. Kerton ◽  
M. J. Alexander ◽  
H. A. Kobulnicky ◽  
B. Uzpen
Keyword(s):  
Mass Star ◽  
Intermediate Mass ◽  
Star Forming ◽  
Star Forming Regions ◽  
Intermediate Mass Star

Intermediate‐Mass Star Models with Different Helium and Metal Contents

2000 ◽  
Vol 543 (2) ◽  
pp. 955-971 ◽  
Author(s):  
Giuseppe Bono ◽  
Filippina Caputo ◽  
Santi Cassisi ◽  
Marcella Marconi ◽  
Luciano Piersanti ◽  
...  
Keyword(s):  
Mass Star ◽  
Intermediate Mass ◽  
Star Models ◽  
Metal Contents ◽  
Intermediate Mass Star
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